Modulation of low energy electrons and protons near solar maximum

Details Modulation of low energy electrons and protons near solar maximum Modulation of low energy electrons and protons near solar maximum

Aug 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975icrc....3..979l&link_type=abstract

In: International Cosmic Ray Conference, 14th, Munich, West Germany, August 15-29, 1975, Conference Papers. Volume 3. (A76-26851

Physics

Cosmic Rays, Electron Energy, Modulation, Particle Intensity, Proton Energy, Solar Activity Effects, Cross Correlation, Forbush Decreases, Magnetic Rigidity, Neutrons, Time Dependence

Scientific paper

The intensities of cosmic-ray electrons in the energy range from 24 to 235 MeV and of protons in the ranges 40 to 150 MeV and greater than 700 MeV are compared with the neutron intensity data over the period 1968 to 1972. Correlation plots between these various components show a marked break following the June 9, 1969 Forbush decrease. The resulting hysteresis curve is best explained as a sudden change in the rigidity dependence of solar modulation. A variation in the size of the solar cavity is also possible but not likely.

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